Metallicity of the star HD80290(F3V)

  • Z. A. Samedov
  • G. M. Hajiyeva
  • Z. F. Aliyeva
  • N.H. Samedova

Abstract

The atmospheres of the HD80290(F3V) star of the F spectral class were studied using the model and parallax methods. The effective temperatures Teff and surface of gravity g of stars were determined based on a comparison of the observed and theoretically calculated values of the photometric quantity [c1] and the equivalent widths of the spectral lines of the hydrogen Balmer series and the use of parallax. Based on the FeII lines, the microturbulence

Published
2022-09-06
How to Cite
SAMEDOV, Z. A. et al. Metallicity of the star HD80290(F3V). Astronomy & Astrophysics (CAUCASUS), [S.l.], v. 5, p. 65-70, sep. 2022. ISSN 2449-2914. Available at: <https://sjunijournals.ge/index.php/AA/article/view/201>. Date accessed: 06 oct. 2022.
Section
Articles